Abstract
The observation of the primary energy spectrum in its energy region of 1016 eV to 1019 eV by using compact Extensive Air Shower (EAS) arrays and the time structure of EAS particles which was studied by Linsley (Linsley method) have been carried out by the Large Area Air Shower group. We have estimated the EAS core distance by using only an EAS array and the Linsley method. To improve the determination accuracy of the primary energy, we consider the estimation method of the core distance by using two EAS arrays (multiple Linsley method). We report on the idea of the multiple Linsley method and the comparison of simulation results in various observation modes.
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